{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:K6LJV2WV3JKA5THWCL6JUUYDPQ","short_pith_number":"pith:K6LJV2WV","schema_version":"1.0","canonical_sha256":"57969aead5da540eccf612fc9a53037c2db4861b8518832356f17ccad188bef0","source":{"kind":"arxiv","id":"1210.4171","version":1},"attestation_state":"computed","paper":{"title":"Molecular gas in the centre of nearby galaxies from VLT/SINFONI integral field spectroscopy - I. Morphology and mass inventory","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"2), (3) Max-Planck-Institut f\\\"ur Physik, Garching, Germany, Germany), Germany (2) Universit\\\"atssternwarte, J. Thomas (1, M. H. Fabricius (1, Michael J. Williams (1) ((1) Max-Planck-Institut f\\\"ur extraterrestrische Physik, M. Opitsch (1), M\\\"unchen, N. Nowak (3), Peter Erwin (1), R. Bender (1, R. P. Saglia (1, S. P. Rusli (1, X. Mazzalay (1)","submitted_at":"2012-10-15T20:00:05Z","abstract_excerpt":"We present the first results of an analysis of the properties of the molecular gas in the nuclear regions (r < 300 pc) of a sample of six nearby galaxies, based on new high spatial resolution observations obtained in the K-band with the near-infrared integral field spectrograph SINFONI at the Very Large Telescope. We derive two-dimensional distributions of the warm molecular and ionized gas from the H2, Br_gamma and HeI emission lines present in the spectra of the galaxies. We find a range of morphologies, including bar- and ring-like distributions and either centrally peaked or off-centre emi"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1210.4171","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-10-15T20:00:05Z","cross_cats_sorted":[],"title_canon_sha256":"903cff213bb322c18c4aae35f78b327ee3d66f503587bace84ddacad936b12e5","abstract_canon_sha256":"3b79cbf484df7ee03a66b04ad1423b654554b4c554e6c259b649b23d69206a2c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:53:54.853233Z","signature_b64":"TIZf9/G1aaSC6Ktk6EhNw88y5q9kk7MmNHjQnvl4VVh9Tu0GaF4XttQwc4AvJvZ4dufxjmlatvvZTJ7mG9rrDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"57969aead5da540eccf612fc9a53037c2db4861b8518832356f17ccad188bef0","last_reissued_at":"2026-05-18T01:53:54.852462Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:53:54.852462Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Molecular gas in the centre of nearby galaxies from VLT/SINFONI integral field spectroscopy - I. Morphology and mass inventory","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"2), (3) Max-Planck-Institut f\\\"ur Physik, Garching, Germany, Germany), Germany (2) Universit\\\"atssternwarte, J. Thomas (1, M. H. Fabricius (1, Michael J. Williams (1) ((1) Max-Planck-Institut f\\\"ur extraterrestrische Physik, M. Opitsch (1), M\\\"unchen, N. Nowak (3), Peter Erwin (1), R. Bender (1, R. P. Saglia (1, S. P. Rusli (1, X. Mazzalay (1)","submitted_at":"2012-10-15T20:00:05Z","abstract_excerpt":"We present the first results of an analysis of the properties of the molecular gas in the nuclear regions (r < 300 pc) of a sample of six nearby galaxies, based on new high spatial resolution observations obtained in the K-band with the near-infrared integral field spectrograph SINFONI at the Very Large Telescope. We derive two-dimensional distributions of the warm molecular and ionized gas from the H2, Br_gamma and HeI emission lines present in the spectra of the galaxies. We find a range of morphologies, including bar- and ring-like distributions and either centrally peaked or off-centre emi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1210.4171","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"1210.4171","created_at":"2026-05-18T01:53:54.852603+00:00"},{"alias_kind":"arxiv_version","alias_value":"1210.4171v1","created_at":"2026-05-18T01:53:54.852603+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1210.4171","created_at":"2026-05-18T01:53:54.852603+00:00"},{"alias_kind":"pith_short_12","alias_value":"K6LJV2WV3JKA","created_at":"2026-05-18T12:27:11.947152+00:00"},{"alias_kind":"pith_short_16","alias_value":"K6LJV2WV3JKA5THW","created_at":"2026-05-18T12:27:11.947152+00:00"},{"alias_kind":"pith_short_8","alias_value":"K6LJV2WV","created_at":"2026-05-18T12:27:11.947152+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/K6LJV2WV3JKA5THWCL6JUUYDPQ","json":"https://pith.science/pith/K6LJV2WV3JKA5THWCL6JUUYDPQ.json","graph_json":"https://pith.science/api/pith-number/K6LJV2WV3JKA5THWCL6JUUYDPQ/graph.json","events_json":"https://pith.science/api/pith-number/K6LJV2WV3JKA5THWCL6JUUYDPQ/events.json","paper":"https://pith.science/paper/K6LJV2WV"},"agent_actions":{"view_html":"https://pith.science/pith/K6LJV2WV3JKA5THWCL6JUUYDPQ","download_json":"https://pith.science/pith/K6LJV2WV3JKA5THWCL6JUUYDPQ.json","view_paper":"https://pith.science/paper/K6LJV2WV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1210.4171&json=true","fetch_graph":"https://pith.science/api/pith-number/K6LJV2WV3JKA5THWCL6JUUYDPQ/graph.json","fetch_events":"https://pith.science/api/pith-number/K6LJV2WV3JKA5THWCL6JUUYDPQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/K6LJV2WV3JKA5THWCL6JUUYDPQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/K6LJV2WV3JKA5THWCL6JUUYDPQ/action/storage_attestation","attest_author":"https://pith.science/pith/K6LJV2WV3JKA5THWCL6JUUYDPQ/action/author_attestation","sign_citation":"https://pith.science/pith/K6LJV2WV3JKA5THWCL6JUUYDPQ/action/citation_signature","submit_replication":"https://pith.science/pith/K6LJV2WV3JKA5THWCL6JUUYDPQ/action/replication_record"}},"created_at":"2026-05-18T01:53:54.852603+00:00","updated_at":"2026-05-18T01:53:54.852603+00:00"}